CORDIS Project
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This project investigates the use of Fast X-ray Transients to study binary neutron star mergers, aiming to understand their role in producing heavy elements and measuring the Hubble constant. It combines observational data from X-ray surveys with theoretical models.
We will use extra-galactic Fast X-ray Transients (FXTs) to study binary neutron star (BNS) mergers.
Merging neutron stars are important for the formation of r-process elements and provide standardizable signals allowing the Hubble constant (H0) to be measured maximizing the science output of these multi-messenger events.
Comparing BNS mergers with and without an FXT signal provides a way to constrain the elusive equation of state of matter at supra-nuclear densities.
Unlike the highly beamed sho…
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